Detection of Dimethyl Ether in the Central Region of the MWC 480 Protoplanetary Disk
Yoshihide Yamato, Yuri Aikawa, Viviana V. Guzm\'an, Kenji Furuya,, Shota Notsu, Gianni Cataldi, Karin I. \"Oberg, Chunhua Qi, Charles J. Law,, Jane Huang, Richard Teague, Romane Le Gal

TL;DR
This study reports the first detection of dimethyl ether in a non-transitional protoplanetary disk, revealing insights into complex organic molecule chemistry during planet formation.
Contribution
It provides the first detection of CH$_3$OCH$_3$ in a non-transitional Class II disk and analyzes its implications for chemical reprocessing in the disk.
Findings
Detection of CH$_3$OCH$_3$ in MWC 480 disk.
High CH$_3$OCH$_3$/CH$_3$OH ratio suggests chemical reprocessing.
COMs likely sublimated in the warm inner disk.
Abstract
Characterizing the chemistry of complex organic molecules (COMs) at the epoch of planet formation provides insights into the chemical evolution of the interstellar medium (ISM) and the origin of organic materials in our Solar System. We report a detection of dimethyl ether (CHOCH) in the disk around the Herbig Ae star MWC 480 with the sensitive Atacama Large Millimeter/submillimeter Array observations. This is the first detection of CHOCH in a non-transitional Class II disk. The spatially unresolved, compact (25 au in radius) nature, the broad line width (30 km s), and the high excitation temperature (200 K) indicate sublimation of COMs in the warm inner disk. Despite the detection of CHOCH, methanol (CHOH), the most abundant COM in the ISM, has not been detected, from which we constrain the column density ratio of…
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Taxonomy
TopicsMolecular Spectroscopy and Structure · Astro and Planetary Science · Astrophysics and Star Formation Studies
